Coronal bright points

Abstract Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray spectrum that connect magnetic flux concentrations of opposite polarities. CBPs are one of the main buildi...

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Bibliografiska uppgifter
Huvudupphovsman: Maria S. Madjarska
Materialtyp: Artikel
Språk:English
Publicerad: Springer 2019-03-01
Serie:Living Reviews in Solar Physics
Ämnen:
Länkar:http://link.springer.com/article/10.1007/s41116-019-0018-8